Evolution of the far-infrared luminosity functions in the Spitzer Wide-area Infrared Extragalactic Legacy Survey

We present new observational determination of the evolution of the rest-frame 70 and 160 micron and total infrared (TIR) galaxy luminosity functions (LFs) using 70 micron data from the Spitzer Wide-area Infrared Extragalactic Legacy Survey (SWIRE). The LFs were constructed for sources with spectroscopic redshifts only in the XMM-LSS and Lockman Hole fields from the SWIRE photometric redshift catalogue. The 70 micron and TIR LFs were constructed in the redshift range 0<z<1.2 and the 160 micron LF was constructed in the redshift range 0<z<0.5 using a parametric Bayesian and the vmax methods. We assume in our models, that the faint-end power-law index of the LF does not evolve with redshifts. We find the the double power-law model is a better representation of the IR LF than the more commonly used power-law and Gaussian model. We model the evolution of the FIR LFs as a function of redshift where where the characteristic luminosity, $L^\ast$ evolve as \propto(1+z)^{\alpha_\textsc{l}}. The rest-frame 70 micron LF shows a strong luminosity evolution out to z=1.2 with alpha_l=3.41^{+0.18}_{-0.25}. The rest-frame 160 micron LF also showed rapid luminosity evolution with alpha_l=5.53^{+0.28}_{-0.23} out to z=0.5. The rate of evolution in luminosity is consistent with values estimated from previous studies using data from IRAS, ISO and Spitzer. The TIR LF evolves in luminosity with alpha_l=3.82^{+0.28}_{-0.16} which is in agreement with previous results from Spitzer 24 micron which find strong luminosity evolution. By integrating the LF we calculated the co-moving IR luminosity density out to z=1.2, which confirm the rapid evolution in number density of LIRGs and ULIRGs which contribute ~68^{+10}_{-07} % to the co-moving star formation rate density at z=1.2. Our results based on 70 micron data confirms that the bulk of the star formation at z=1 takes place in dust obscured objects.Comment: 17 pages, 14 figure

Infrared Constraints on AGN Tori Models

This work focuses on the properties of dusty tori in active galactic nuclei (AGN) derived from the comparison of SDSS type 1 quasars with mid-Infrared (MIR) counterparts and a new, detailed torus model. The infrared data were taken by the Spitzer Wide-area InfraRed Extragalactic (SWIRE) Survey. Basic model parameters are constraint, such as the density law of the graphite and silicate grains, the torus size and its opening angle. A whole variety of optical depths is supported. The favoured models are those with decreasing density with distance from the centre, while there is no clear tendency as to the covering factor, ie small, medium and large covering factors are almost equally distributed. Based on the models that better describe the observed SEDs, properties such as the accretion luminosity, the mass of dust, the inner to outer radius ratio and the hydrogen column density are computed.Comment: 4 pages, 4 figures, to appear in "Infrared Diagnostics of Galaxy Evolution", ASP Conference Series, Pasadena, 14-16 November 200

Near-Infrared and Star-forming properties of Local Luminous Infrared Galaxies

We use HST NICMOS continuum and Pa-alpha observations to study the near-infrared and star-formation properties of a representative sample of 30 local (d ~ 35-75Mpc) luminous infrared galaxies (LIRGs, infrared 8-1000um luminosities of L_IR=11-11.9[Lsun]). The data provide spatial resolutions of 25-50pc and cover the central ~3.3-7.1kpc regions of these galaxies. About half of the LIRGs show compact (~1-2kpc) Pa-alpha emission with a high surface brightness in the form of nuclear emission, rings, and mini-spirals. The rest of the sample show Pa-alpha emission along the disk and the spiral arms extending over scales of 3-7kpc and larger. About half of the sample contains HII regions with H-alpha luminosities significantly higher than those observed in normal galaxies. There is a linear empirical relationship between the mid-IR 24um and hydrogen recombination (extinction-corrected Pa-alpha) luminosity for these LIRGs, and the HII regions in the central part of M51. This relation holds over more than four decades in luminosity suggesting that the mid-IR emission is a good tracer of the star formation rate (SFR). Analogous to the widely used relation between the SFR and total IR luminosity of Kennicutt (1998), we derive an empirical calibration of the SFR in terms of the monochromatic 24um luminosity that can be used for luminous, dusty galaxies.Comment: Accepted for publication in ApJ. Contact first author for high qualitity version of figure

Chronic environmental perturbation influences microbial community assembly patterns

Acknowledgements Next-generation sequencing and library construction was performed by NCIMB Ltd., Aberdeen and CGEBM, Aberdeen. The authors would like to acknowledge the support of the Maxwell computer cluster funded by the University of Aberdeen. Dr Axel Aigle is acknowledged for assistance in molecular analysis. This work was supported by the Natural Environment Research Council [NE/L00982X/1] with financial support from BP UK Ltd and Intertek Group PLC. CGR was supported by a University Research Fellowship from the Royal Society [UF150571]Peer reviewedPostprin

Variación estacional en escarabajos coprofagos (coleoptera: scarabaeidae: scarabaeinae) de la serranía de coraza, sucre (colombia)

This study presents the seasonal variation of data collected from observation of a dung beetle community living in an area of tropical dry forest, with another living in an area used for cattle raising, which is located in the Serranía de Corozá Colosó – Sucre. Over the course of one year - from March 2008 until March 2009 - data was collected using pitfall traps and flight interception. Both of these were left in the field for periods of 48 hours. Some hand capture methods were also used to accomplish a collection of 14 samples. We observed a total of 7496 specimens, representing 26 species. The analysis showed positive correlations between precipitation, richness and abundance of the sites sampled, excepting the abundance in the forest zone, which was positive but not significantEn este estudio se presenta la variación estacional de escarabajos coprófagos en un relicto de bosque seco tropical y una zona de uso ganadero localizadas en la Serranía de Coraza, Colosó – Sucre. Para ello, se realizaron 14 muestreos, entre marzo de 2008 y marzo de 2009, utilizando trampas de caída cebadas, trampas de interceptación de vuelo y colecta manual, dejadas por un periodo de 48 horas en campo. En total se capturaron 7496 individuos pertenecientes a 26 especies. Se verificó correlaciones positivas entre la precipitación mensual, la riqueza y abundancia de individuos, exceptuando la abundancia para la zona boscosa cuya correlación es positiva pero no significativa

Listado de escarabajos coprofagos (coleoptera: scarabaeidae: scarabaeinae) de la serrania de coraza, sucre (colombia)

This study presents the preliminary list of data collected from observation of a dung beetle community living in an area of tropical dry forest, with another living in an area used for cattle raising, which is located in the Serranía de Corozá Colosó – Sucre. Over the course of one year - from March 2008 until March 2009 - data was collected using pitfall traps and flight interception. Both of these were left in the field for periods of 48 hours. Some hand capture methods were also used to accomplish a collection of 14 samples. We observed a total of 7496 specimens, representing 26 species and 14 genera.En este estudio se presenta el listado preliminar de escarabajos coprófagos en un relicto de bosque seco tropical y una zona de uso ganadero localizadas en la Serranía de Coraza, Colosó – Sucre. Para ello, se realizaron 14 muestreos, entre marzo de 2008 y marzo de 2009, utilizando trampas de caída cebadas, trampas de interceptación de vuelo y colecta manual. En total se capturaron 7496 individuos pertenecientes a 26 especies y 14 géneros

Selection of extreme phenotypes: the role of clinical observation in translational research

Systematic collection of phenotypes and their correlation with molecular data has been proposed as a useful method to advance in the study of disease. Although some databases for animal species are being developed, progress in humans is slow, probably due to the multifactorial origin of many human diseases and to the intricacy of accurately classifying phenotypes, among other factors. An alternative approach has been to identify and to study individuals or families with very characteristic, clinically relevant phenotypes. This strategy has shown increased efficiency to identify the molecular features underlying such phenotypes. While on most occasions the subjects selected for these studies presented harmful phenotypes, a few studies have been performed in individuals with very favourable phenotypes. The consistent results achieved suggest that it seems logical to further develop this strategy as a methodology to study human disease, including cancer. The identification and the study with high-throughput techniques of individuals showing a markedly decreased risk of developing cancer or of cancer patients presenting either an unusually favourable prognosis or striking responses following a specific treatment, might be promising ways to maximize the yield of this approach and to reveal the molecular causes that explain those phenotypes and thus highlight useful therapeutic targets. This manuscript reviews the current status of selection of extreme phenotypes in cancer research and provides directions for future development of this methodology

Design of a polishing tool for collaborative robotics using minimum viable product approach

This is an Author's Accepted Manuscript of an article published in Carlos Perez-Vidal, Luis Gracia, Samuel Sanchez-Caballero, J. Ernesto Solanes, Alessandro Saccon & Josep Tornero (2019) Design of a polishing tool for collaborative robotics using minimum viable product approach, International Journal of Computer Integrated Manufacturing, 32:9, 848-857, DOI: 10.1080/0951192X.2019.1637026 [copyright Taylor & Francis], available online at: http://www.tandfonline.com/10.1080/0951192X.2019.1637026[EN] A collaborative tool for robotic polishing is developed in this work in order to allow the simultaneous operation of the robot system and human operator to cooperatively carry out the polishing task. For this purpose, the collaborative environment is detailed and the polishing application is designed. Moreover, the polishing tool is developed and its implementation using the minimum viable product approach is obtained. Furthermore, a robust hybrid position-force control is proposed to use the developed tool attached to a robot system and some experiments are given to show its performance.This work was supported in part by the Ministerio de Ciencia e Innovacion (Spanish Government) under project [DPI2017-87656-C2-1-R] and the Generalitat Valenciana under Grant [VALi+ d APOSTD/2016/044].Perez-Vidal, C.; Gracia Calandin, LI.; Sanchez-Caballero, S.; Solanes Galbis, JE.; Saccon, A.; Tornero Montserrat, J. (2019). Design of a polishing tool for collaborative robotics using minimum viable product approach. International Journal of Computer Integrated Manufacturing. 32(9):848-857. https://doi.org/10.1080/0951192X.2019.1637026S848857329Alders, K., M. Lehe, and G. 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